Fission Fragment Distribution and the r-Process

Exotic Nuclei ◽  
2019 ◽  
Author(s):  
I. V. Panov ◽  
I. Yu. Korneev
2021 ◽  
Vol 103 (2) ◽  
Author(s):  
J.-F. Lemaître ◽  
S. Goriely ◽  
A. Bauswein ◽  
H.-T. Janka

1992 ◽  
Vol 343 (1) ◽  
pp. 73-77 ◽  
Author(s):  
H. Machner ◽  
Sa Jun ◽  
G. Riepe ◽  
D. Protic ◽  
H. Daniel ◽  
...  

2008 ◽  
Author(s):  
S. Chiba ◽  
H. Koura ◽  
T. Maruyama ◽  
M. Ohta ◽  
S. Tatsuda ◽  
...  

2018 ◽  
Vol 169 ◽  
pp. 00011
Author(s):  
Vitaly Khryachkov ◽  
Andrei Goverdovskii ◽  
Vladimir Ketlerov ◽  
Vecheslav Mitrofanov ◽  
Alexei Sergachev

Binary fission of 232Th and 238U induced by fast neutrons were under intent investigation in the IPPE during recent years. These measurements were performed with a twin ionization chamber with Frisch grids. Signals from the detector were digitized for further processing with a specially developed software. It results in information of kinetic energies, masses, directions and Bragg curves of registered fission fragments. Total statistics of a few million fission events were collected during each experiment. It was discovered that for several combinations of fission fragment masses their total kinetic energy was very close to total free energy of the fissioning system. The probability of such fission events for the fast neutron induced fission was found to be much higher than for spontaneous fission of 252Cf and thermal neutron induced fission of 235U. For experiments with 238U target the energy of incident neutrons were 5 MeV and 6.5 MeV. Close analysis of dependence of fission fragment distribution on compound nucleus excitation energy gave us some explanation of the phenomenon. It could be a process in highly excited compound nucleus which leads the fissioning system from the scission point into the fusion valley with high probability.


2020 ◽  
Vol 242 ◽  
pp. 04002
Author(s):  
Nicole Vassh ◽  
Matthew Mumpower ◽  
Trevor Sprouse ◽  
Rebecca Surman ◽  
Ramona Vogt

We review recent work examining the influence of fission in rapid neutron capture (r-process) nucleosynthesis which can take place in astrophysical environments. We briefly discuss the impact of uncertain fission barriers and fission rates on the population of heavy actinide species. We demonstrate the influence of the fission fragment distributions for neutron-rich nuclei and discuss currently available treatments, including recent macroscopic-microscopic calculations. We conclude by comparing our nucleosynthesis results directly with stellar data for metal-poor stars rich in r-process elements to consider whether fission plays a role in the so-called ‘universality’ of r-process abundances observed from star to star.


2020 ◽  
Vol 101 (6) ◽  
Author(s):  
Jhilam Sadhukhan ◽  
Samuel A. Giuliani ◽  
Zachary Matheson ◽  
Witold Nazarewicz

2009 ◽  
Vol 33 (S1) ◽  
pp. 119-122
Author(s):  
Wang Kun ◽  
Ma Yu-Gang ◽  
Zheng Qing-Shan ◽  
Cai Xiang-Zhou ◽  
Fang De-Qing ◽  
...  

2007 ◽  
Author(s):  
S. Tatsuda ◽  
K. Hashizume ◽  
T. Wada ◽  
M. Ohta ◽  
K. Sumiyoshi ◽  
...  

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